Timescales of Solar System Formation Based on Al–Ti Isotope Correlation by Supernova Ejecta
The radioactive decay of short-lived ^26 Al– ^26 Mg has been used to estimate the timescales over which ^26 Al was produced in a nearby star and the protosolar disk evolved. The chronology commonly assumes that ^26 Al was uniformly distributed in the protosolar disk; however, this assumption is chal...
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Main Authors: | Tsuyoshi Iizuka, Yuki Hibiya, Satoshi Yoshihara, Takehito Hayakawa |
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Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
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Series: | The Astrophysical Journal Letters |
Subjects: | |
Online Access: | https://doi.org/10.3847/2041-8213/ada554 |
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